collaborators

8 papers

astro-ph.HE2026

Constraints on Line-of-Sight Acceleration from O1-O4

Labani Roy, Alexander H. Nitz

A compact binary will experience a center-of-mass (CoM) acceleration in the vicinity of a massive third object. The line-of-sight (LOS) component of this acceleration is imprinted…

astro-ph.HE2026

Las Cumbres Observatory Gravitational-Wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy

Ido Keinan, Iair Arcavi, D. Andrew Howell +34

We present a summary of gravitational-wave (GW) follow-up using the Las Cumbres Observatory global network of telescopes during the third (O3) and fourth (O4) observing runs of the…

astro-ph.HE2026

Search for Sub-Solar Mass Binaries in the First Part of LIGO's Fourth Observing Run

Keisi Kacanja, Kanchan Soni, Aleyna Akyüz +1

We report the first results of a sub-solar mass compact binary search using the data from the first part of the fourth observing run (O4a) of the Advanced LIGO detectors. Sub-solar…

astro-ph.IM2026

Beyond FINDCHIRP: Breaking the memory wall and optimal FFTs for Gravitational-Wave Matched-Filter Searches with Ratio-Filter Dechirping

Alexander H. Nitz, Keisi Kacanja, Kanchan Soni

A primary bottleneck in modern FFT-based matched-filter searches for gravitational waves from compact binary coalescences is not raw processor throughput, but available memory band…

gr-qc2025

Eccentricity signatures in LIGO-Virgo-KAGRA's BNS and NSBH binaries

Keisi Kacanja, Kanchan Soni, Alexander Harvey Nitz

Measurement of eccentricity in low-mass binary systems through gravitational waves is crucial to distinguish between various formation channels. Detecting eccentricity in these sys…

gr-qc2025

Potential science with GW250114 -- the loudest binary black hole merger detected to date

Aleyna Akyüz, Alex Correia, Jada Garofalo +7

On January 14, 2025 the LIGO interferometers detected a gravitational wave from the merger of two black holes, GW250114. Using publicly available information, we estimate that the…